Growth and characterization of B-InN films on MgO: the key role of a B-GaN buffer layer in growing cubic InN
Cubic InN samples were grown on MgO (001) substrates by gas source molecular beam epitaxy (GSMBE). In general, we find that InN directly deposited onto the MgO substrate results in polycrystalline or columnar films of hexagonal symmetry. We find that adequateconditions to grow the cubic phase of thi...
| Autores: | , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2012 |
| País: | México |
| Institución: | Universidad Autónoma de San Luis Potosí |
| Repositorio: | Redalyc-UASLP |
| OAI Identifier: | oai:redalyc.org:57023422005 |
| Acceso en línea: | https://www.redalyc.org/articulo.oa?id=57023422005 |
| Access Level: | acceso abierto |
| Palabra clave: | Física, Astronomía y Matemáticas A3 B2 B1 nitrides V materials |
| Sumario: | Cubic InN samples were grown on MgO (001) substrates by gas source molecular beam epitaxy (GSMBE). In general, we find that InN directly deposited onto the MgO substrate results in polycrystalline or columnar films of hexagonal symmetry. We find that adequateconditions to grow the cubic phase of this compound require the growth of an initial cubic GaN buffer interlayer (¿-tGaN) on the MgO surface. Subsequently, the growth conditions were optimized to obtain good photoluminescence (PL) emission. The resultant InN growthis mostly cubic, with very small hexagonal inclusions, as confirmed by X-ray diffraction (XRD) and scanning electron microscopy (SEM) studies. Good crystalline quality requires that the samples to be grown under rich Indium metal flux. The cubic ¿-tInN/GaN/MgO samplesexhibit a high signal to noise ratio for PL at low temperatures (20 K). The PL is centered at 0.75 eV and persists at room temperature. |
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